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Under stable atmospheric conditions, the zenithal brightness of the urban sky varies throughout the night following the time course of the anthropogenic emissions of light. Different types of artificial light sources (e.g. streetlights,…

Instrumentation and Methods for Astrophysics · Physics 2018-11-12 Salvador Bará , Ángel Rodríguez-Arós , Marcos Pérez , Borja Tosar , Raul C. Lima , Alejandro Sánchez de Miguel , Jaime Zamorano

Modeling the hemispherical night sky brightness of anthropogenic origin is a demanding computational challenge, due to the intensive calculations required to produce all-sky maps with fine angular resolution including high-order scattering…

Instrumentation and Methods for Astrophysics · Physics 2022-03-30 Miroslav Kocifaj , Salvador Bará , Fabio Falchi

The visual perception of the natural night sky in many places of the world is strongly disturbed by anthropogenic light. Part of this artificial light is scattered in the atmosphere and propagates towards the observer, adding to the natural…

Instrumentation and Methods for Astrophysics · Physics 2023-05-02 Salvador Bará , Carmen Bao-Varela

Nighttime monitoring of the aerosol content of the lower atmosphere is a challenging task, because appropriate reference natural light sources are lacking. Here we show that the anthropogenic night sky brightness due to city lights can be…

Instrumentation and Methods for Astrophysics · Physics 2020-11-18 Miroslav Kocifaj , Salvador Bará

Measuring the brightness of the night sky has become an increasingly important topic in recent years, as artificial lights and their scattering by the Earths atmosphere continue spreading around the globe. Several instruments and techniques…

The population of artificial satellites and space debris orbiting the Earth imposes non-negligible constraints on both space operations and ground-based optical and radio astronomy. The ongoing deployment of several satellite…

Instrumentation and Methods for Astrophysics · Physics 2021-04-02 Miroslav Kocifaj , Frantisek Kundracik , John C. Barentine , Salvador Bará

We present a method to map the artificial sky brightness across large territories in astronomical photometric bands with a resolution of approximately 1 km. This is useful to quantify the situation of night sky pollution, to recognize…

Astrophysics · Physics 2009-10-31 P. Cinzano , F. Falchi , C. D. Elvidge , K. E. Baugh

Ground-based optical astronomy necessarily involves sensing the light of astronomical objects along with the contributions of many natural sources ranging from the Earth's atmosphere to cosmological light. In addition, astronomers have long…

Instrumentation and Methods for Astrophysics · Physics 2022-08-31 John C. Barentine

Determining the all-sky radiance distribution produced by artificial light sources is a computationally demanding task that generally requires an intensive calculation load. We develop in this work an analytic formulation that provides the…

Instrumentation and Methods for Astrophysics · Physics 2019-10-24 Miroslav Kocifaj , Salvador Bará

The knowledge of the contribution $b_d(d)$ to the artificial sky luminance in a given point of the sky of a site produced by the sources beyond a given distance $d$ from it is important to understand the behaviour of light pollution in…

Astrophysics · Physics 2007-05-23 P. Cinzano

Estimating the horizontal irradiance from measurements of the zenith night sky radiance is a useful operation for basic and applied studies in observatory site assessment, atmospheric optics and environmental sciences. The ratio between…

Instrumentation and Methods for Astrophysics · Physics 2022-02-16 Salvador Bará , Xabier Pérez-Couto , Fabio Falchi , Miroslav Kocifaj , Eduard Masana

The direction of the upward light emission has different polluting effects on the sky depending on the distance of the observation site. We studied with detailed models for light pollution propagation the ratio $(b_{H})/(b_{L})$, at given…

Astrophysics · Physics 2007-05-23 P. Cinzano , F. J. Diaz Castro

We apply the sky brightness modelling technique introduced and developed by Roy Garstang to high-resolution DMSP-OLS satellite measurements of upward artificial light flux and to GTOPO30 digital elevation data in order to predict the…

Astrophysics · Physics 2009-11-10 Pierantonio Cinzano , Cristopher D. Elvidge

We obtained the map of the zenith brightness of the night sky in Italy. The artificial sky brightness in each site is computed by integration of the contributions by each unitary area of surface obtained by applying a propagation function…

Astrophysics · Physics 2007-05-23 F. Falchi , P. Cinzano

We report on luminance measurements of the summer night sky at a field site on a freshwater lake in northeastern Germany (Lake Stechlin) to evaluate the amount of artificial skyglow from nearby and distant towns in the context of a planned…

Solar and Stellar Astrophysics · Physics 2016-02-16 Andreas Jechow , Franz Hölker , Zoltán Kolláth , Mark O. Gessner , Christopher C. M. Kyba

A recurring question arises when trying to characterize, by means of measurements or theoretical calculations, the zenithal night sky brightness throughout a large territory: how many samples per square kilometer are needed? The optimum…

Instrumentation and Methods for Astrophysics · Physics 2018-11-12 Salvador Bará

We present the map of the artificial sky brightness in Europe in V band with a resolution of approximately 1 km. The aim is to understand the state of night sky pollution in Europe, to quantify the present situation and to allow future…

Astrophysics · Physics 2007-05-23 P. Cinzano , F. Falchi , C. D. Elvidge , K. E. Baugh

Artificial skyglow is a form of light pollution with wide ranging implications on the environment. The extent, intensity and color of skyglow depends on the artificial light sources and weather conditions. Skyglow can be best determined…

Instrumentation and Methods for Astrophysics · Physics 2022-02-17 Andreas Jechow , Christopher C. M. Kyba , Franz Hölker

We present the first World Atlas of the zenith artificial night sky brightness at sea level. Based on radiance calibrated high resolution DMSP satellite data and on accurate modelling of light propagation in the atmosphere, it provides a…

Astrophysics · Physics 2009-11-07 P. Cinzano , F. Falchi , C. D. Elvidge

Modelling techniques for the propagation of light pollution in the atmosphere allow the computation of maps of artificial night sky brightness in any direction of the sky, involving a large number of details from satellite data. Cinzano et…

Instrumentation and Methods for Astrophysics · Physics 2020-07-02 Pierantonio Cinzano , Fabio Falchi
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